There are many ways to derive the
Lorentz transformation
In physics, the Lorentz transformations are a six-parameter family of Linear transformation, linear coordinate transformation, transformations from a Frame of Reference, coordinate frame in spacetime to another frame that moves at a constant vel ...
s using a variety of physical principles, ranging from
Maxwell's equations
Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, Electrical network, electr ...
to Einstein's
postulates of special relativity, and
mathematical
Mathematics is a field of study that discovers and organizes methods, Mathematical theory, theories and theorems that are developed and Mathematical proof, proved for the needs of empirical sciences and mathematics itself. There are many ar ...
tools, spanning from
elementary algebra
Elementary algebra, also known as high school algebra or college algebra, encompasses the basic concepts of algebra. It is often contrasted with arithmetic: arithmetic deals with specified numbers, whilst algebra introduces variable (mathematics ...
and
hyperbolic function
In mathematics, hyperbolic functions are analogues of the ordinary trigonometric functions, but defined using the hyperbola rather than the circle. Just as the points form a circle with a unit radius, the points form the right half of the ...
s, to
linear algebra
Linear algebra is the branch of mathematics concerning linear equations such as
:a_1x_1+\cdots +a_nx_n=b,
linear maps such as
:(x_1, \ldots, x_n) \mapsto a_1x_1+\cdots +a_nx_n,
and their representations in vector spaces and through matrix (mathemat ...
and
group theory
In abstract algebra, group theory studies the algebraic structures known as group (mathematics), groups.
The concept of a group is central to abstract algebra: other well-known algebraic structures, such as ring (mathematics), rings, field ( ...
.
This article provides a few of the easier ones to follow in the context of
special relativity
In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between Spacetime, space and time. In Albert Einstein's 1905 paper, Annus Mirabilis papers#Special relativity,
"On the Ele ...
, for the simplest case of a Lorentz boost in standard configuration, i.e. two
inertial frame
In classical physics and special relativity, an inertial frame of reference (also called an inertial space or a Galilean reference frame) is a frame of reference in which objects exhibit inertia: they remain at rest or in uniform motion relative ...
s moving relative to each other at constant (uniform)
relative velocity less than the
speed of light
The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
, and using
Cartesian coordinates
In geometry, a Cartesian coordinate system (, ) in a plane is a coordinate system that specifies each point uniquely by a pair of real numbers called ''coordinates'', which are the signed distances to the point from two fixed perpendicular o ...
so that the ''x'' and ''x''′ axes are
collinear
In geometry, collinearity of a set of Point (geometry), points is the property of their lying on a single Line (geometry), line. A set of points with this property is said to be collinear (sometimes spelled as colinear). In greater generality, t ...
.
Lorentz transformation
In the fundamental branches of
modern physics
Modern physics is a branch of physics that developed in the early 20th century and onward or branches greatly influenced by early 20th century physics. Notable branches of modern physics include quantum mechanics, special relativity, and genera ...
, namely
general relativity
General relativity, also known as the general theory of relativity, and as Einstein's theory of gravity, is the differential geometry, geometric theory of gravitation published by Albert Einstein in 1915 and is the current description of grav ...
and its widely applicable subset
special relativity
In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between Spacetime, space and time. In Albert Einstein's 1905 paper, Annus Mirabilis papers#Special relativity,
"On the Ele ...
, as well as
relativistic quantum mechanics and
relativistic quantum field theory
In theoretical physics, quantum field theory (QFT) is a theoretical framework that combines field theory and the principle of relativity with ideas behind quantum mechanics. QFT is used in particle physics to construct physical models of suba ...
, the
Lorentz transformation
In physics, the Lorentz transformations are a six-parameter family of Linear transformation, linear coordinate transformation, transformations from a Frame of Reference, coordinate frame in spacetime to another frame that moves at a constant vel ...
is the transformation rule under which all
four-vector
In special relativity, a four-vector (or 4-vector, sometimes Lorentz vector) is an object with four components, which transform in a specific way under Lorentz transformations. Specifically, a four-vector is an element of a four-dimensional vect ...
s and
tensor
In mathematics, a tensor is an algebraic object that describes a multilinear relationship between sets of algebraic objects associated with a vector space. Tensors may map between different objects such as vectors, scalars, and even other ...
s containing
physical quantities
A physical quantity (or simply quantity) is a property of a material or system that can be quantified by measurement. A physical quantity can be expressed as a ''value'', which is the algebraic multiplication of a '' numerical value'' and a '' ...
transform from one
frame of reference
In physics and astronomy, a frame of reference (or reference frame) is an abstract coordinate system, whose origin (mathematics), origin, orientation (geometry), orientation, and scale (geometry), scale have been specified in physical space. It ...
to another.
The prime examples of such four-vectors are the
four-position and
four-momentum
In special relativity, four-momentum (also called momentum–energy or momenergy) is the generalization of the classical three-dimensional momentum to four-dimensional spacetime. Momentum is a vector in three dimensions; similarly four-momentum i ...
of a
particle
In the physical sciences, a particle (or corpuscle in older texts) is a small localized object which can be described by several physical or chemical properties, such as volume, density, or mass.
They vary greatly in size or quantity, from s ...
, and for
fields the
electromagnetic tensor and
stress–energy tensor. The fact that these objects transform according to the Lorentz transformation is what mathematically ''defines'' them as vectors and tensors; see
tensor
In mathematics, a tensor is an algebraic object that describes a multilinear relationship between sets of algebraic objects associated with a vector space. Tensors may map between different objects such as vectors, scalars, and even other ...
for a definition.
Given the components of the four-vectors or tensors in some frame, the "transformation rule" allows one to determine the altered components of the same four-vectors or tensors in another frame, which could be boosted or accelerated, relative to the original frame. A "boost" should not be conflated with
spatial translation, rather it's characterized by the
relative velocity between frames. The transformation rule itself depends on the relative motion of the frames. In the simplest case of two
inertial frame
In classical physics and special relativity, an inertial frame of reference (also called an inertial space or a Galilean reference frame) is a frame of reference in which objects exhibit inertia: they remain at rest or in uniform motion relative ...
s the relative velocity between enters the transformation rule. For
rotating reference frame
A rotating frame of reference is a special case of a non-inertial reference frame that is rotation, rotating relative to an inertial reference frame. An everyday example of a rotating reference frame is the surface of the Earth. (This article co ...
s or general
non-inertial reference frames, more parameters are needed, including the relative velocity (magnitude and direction), the rotation axis and angle turned through.
Historical background
The usual treatment (e.g.,
Albert Einstein
Albert Einstein (14 March 187918 April 1955) was a German-born theoretical physicist who is best known for developing the theory of relativity. Einstein also made important contributions to quantum mechanics. His mass–energy equivalence f ...
's original work) is based on the invariance of the speed of light. However, this is not necessarily the starting point: indeed (as is described, for example, in the second volume of the ''
Course of Theoretical Physics'' by
Landau
Landau (), officially Landau in der Pfalz (, ), is an autonomous (''kreisfrei'') town surrounded by the Südliche Weinstraße ("Southern Wine Route") district of southern Rhineland-Palatinate, Germany. It is a university town (since 1990), a long ...
and
Lifshitz), what is really at stake is the
''locality'' of interactions: one supposes that the influence that one particle, say, exerts on another can not be transmitted instantaneously. Hence, there exists a theoretical maximal speed of information transmission which must be invariant, and it turns out that this speed coincides with the speed of light in vacuum.
Newton had himself called the idea of action at a distance philosophically "absurd", and held that gravity had to be transmitted by some agent according to certain laws.
Michelson and
Morley in 1887 designed an experiment, employing an interferometer and a half-silvered mirror, that was accurate enough to detect
aether flow. The mirror system reflected the light back into the interferometer. If there were an
aether drift, it would produce a phase shift and a change in the interference that would be detected. However, no phase shift was ever found. The negative outcome of the
Michelson–Morley experiment
The Michelson–Morley experiment was an attempt to measure the motion of the Earth relative to the luminiferous aether, a supposed medium permeating space that was thought to be the carrier of light waves. The experiment was performed between ...
left the concept of aether (or its drift) undermined. There was consequent perplexity as to why light evidently behaves like a wave, without any detectable medium through which wave activity might propagate.
In a 1964 paper,
Erik Christopher Zeeman showed that the
causality-preserving property, a condition that is weaker in a mathematical sense than the invariance of the speed of light, is enough to assure that the coordinate transformations are the Lorentz transformations. Norman Goldstein's paper shows a similar result using ''inertiality'' (the preservation of time-like lines) rather than ''causality''.
Physical principles
Einstein based his theory of special relativity on two fundamental postulates. First, all physical laws are the same for all inertial frames of reference, regardless of their relative state of motion; and second, the speed of light in free space is the same in all inertial frames of reference, again, regardless of the relative velocity of each reference frame. The Lorentz transformation is fundamentally a direct consequence of this second postulate.
The second postulate
Assume the
second postulate of special relativity stating the constancy of the speed of light, independent of reference frame, and consider a collection of reference systems moving with respect to each other with constant velocity, i.e.
inertial systems, each endowed with its own set of
Cartesian coordinates
In geometry, a Cartesian coordinate system (, ) in a plane is a coordinate system that specifies each point uniquely by a pair of real numbers called ''coordinates'', which are the signed distances to the point from two fixed perpendicular o ...
labeling the points, i.e.
events of spacetime. To express the invariance of the speed of light in mathematical form, fix two events in spacetime, to be recorded in each reference frame. Let the first event be the emission of a light signal, and the second event be it being absorbed.
Pick any reference frame in the collection. In its coordinates, the first event will be assigned coordinates
, and the second
. The spatial distance between emission and absorption is
, but this is also the distance
traveled by the signal. One may therefore set up the equation
Every other coordinate system will record, in its own coordinates, the same equation. This is the immediate mathematical consequence of the invariance of the speed of light. The quantity on the left is called the ''
spacetime interval''. The interval is, for events separated by light signals, the same (zero) in all reference frames, and is therefore called ''
invariant''.
Invariance of interval
For the Lorentz transformation to have the physical significance realized by nature, it is crucial that the interval is an invariant measure for ''any'' two events, not just for those separated by light signals. To establish this, one considers an ''infinitesimal'' interval,
as recorded in a system
. Let
be another system assigning the interval
to the same two infinitesimally separated events. Since if
, then the interval will also be zero in any other system (second postulate), and since
and
are infinitesimals of the same order, they must be proportional to each other,
On what may
depend? It may not depend on the positions of the two events in spacetime, because that would violate the postulated ''homogeneity of spacetime''. It might depend on the relative velocity
between
and
, but only on the speed, not on the direction, because the latter would violate the ''isotropy of space''.
Now bring in systems
and
,
From these it follows,
Now, one observes that on the right-hand side that
depend on both
and
; as well as on the angle between the ''vectors''
and
. However, one also observes that the left-hand side does not depend on this angle. Thus, the only way for the equation to hold true is if the function
is a constant. Further, by the same equation this constant is unity. Thus,
for all systems
. Since this holds for all infinitesimal intervals, it holds for ''all'' intervals.
Most, if not all, derivations of the Lorentz transformations take this for granted. In those derivations, they use the constancy of the speed of light (invariance of light-like separated events) only. This result ensures that the Lorentz transformation is the correct transformation.
Rigorous Statement and Proof of Proportionality of ''ds''2 and ''ds''′2
Theorem:
Let
be integers,
and
a
vector space
In mathematics and physics, a vector space (also called a linear space) is a set (mathematics), set whose elements, often called vector (mathematics and physics), ''vectors'', can be added together and multiplied ("scaled") by numbers called sc ...
over
of
dimension
In physics and mathematics, the dimension of a mathematical space (or object) is informally defined as the minimum number of coordinates needed to specify any point within it. Thus, a line has a dimension of one (1D) because only one coo ...
. Let
be an indefinite-inner product on
with
signature
A signature (; from , "to sign") is a depiction of someone's name, nickname, or even a simple "X" or other mark that a person writes on documents as a proof of identity and intent. Signatures are often, but not always, Handwriting, handwritt ...
type
. Suppose
is a symmetric bilinear form on
such that the null set of the
associated quadratic form of
is contained in that of
(i.e. suppose that for every
, if
then
). Then, there exists a constant
such that
. Furthermore, if we assume
and that
also has signature type
, then we have
.
Remarks.
* In
the section above, the term "infinitesimal" in relation to
is actually referring (pointwise) to a
quadratic form
In mathematics, a quadratic form is a polynomial with terms all of degree two (" form" is another name for a homogeneous polynomial). For example,
4x^2 + 2xy - 3y^2
is a quadratic form in the variables and . The coefficients usually belong t ...
over a four-dimensional real vector space (namely the
tangent space
In mathematics, the tangent space of a manifold is a generalization of to curves in two-dimensional space and to surfaces in three-dimensional space in higher dimensions. In the context of physics the tangent space to a manifold at a point can be ...
at a point of the spacetime manifold). The argument above is copied almost verbatim from Landau and Lifshitz, where the proportionality of
and
is merely stated as an 'obvious' fact even though the statement is not formulated in a mathematically precise fashion nor proven. This is a non-obvious mathematical fact which needs to be justified; fortunately the proof is relatively simple and it amounts to basic algebraic observations and manipulations.
* The above assumptions on
means the following:
is a
bilinear form
In mathematics, a bilinear form is a bilinear map on a vector space (the elements of which are called '' vectors'') over a field ''K'' (the elements of which are called '' scalars''). In other words, a bilinear form is a function that is linea ...
which is symmetric and
non-degenerate, such that there exists an ordered
basis of
for which
An equivalent way of saying this is that
has the matrix representation
relative to the ordered basis
.
* If we consider the special case where
then we're dealing with the situation of
Lorentzian signature in 4-dimensions, which is what relativity is based on (or one could adopt the opposite convention with an overall minus sign; but this clearly doesn't affect the truth of the theorem). Also, in this case, if we assume
and
both have quadratics forms with the same null-set (in physics terminology, we say that
and
give rise to the same light cone) then the theorem tells us that there is a constant
such that
. Modulo some differences in notation, this is precisely what was used in
the section above.
Proof of Theorem.
Fix a basis
of
relative to which
has the matrix representation
. The point is that the vector space
can be decomposed
into subspaces
(the span of the first
basis vectors) and
(then span of the other
basis vectors) such that each vector in
can be written uniquely as
for
and
; moreover
,
and
. So (by bilinearity)
Since the first summand on the right in non-positive and the second in non-negative, for any
and
, we can find a scalar
such that
.
From now on, always consider
and
. By bilinearity
If
, then also
and the same is true for
(since the null-set of
is contained in that of
). In that case, subtracting the two expression above (and dividing by 4) yields
As above, for each
and
, there is a scalar
such that
, so
, which by bilinearity means
.
Now consider nonzero
such that
. We can find
such that
. By the expressions above,
Analogically, for
, one can show that if
, then also
. So it holds for all vectors in
.
For
, if
,
for some
, we can (scaling one of the if necessary) assume
, which by the above means that
. So
.
Finally, if we assume that
both have signature types
and
then
(we can't have
because that would mean
, which is impossible since having signature type
means it is a non-zero bilinear form. Also, if
, then it means
has
positive diagonal entries and
negative diagonal entries; i.e. it is of signature
, since we assumed
, so this is also not possible. This leaves us with
as the only option). This completes the proof of the theorem.
Standard configuration

The invariant interval can be seen as a non-positive definite distance function on spacetime. The set of transformations sought must leave this distance invariant. Due to the reference frame's coordinate system's cartesian nature, one concludes that, as in the Euclidean case, the possible transformations are made up of translations and rotations, where a slightly broader meaning should be allowed for the term rotation.
The interval is quite trivially invariant under translation. For rotations, there are four coordinates. Hence there are six planes of rotation. Three of those are rotations in spatial planes. The interval is invariant under ordinary rotations too.
[
It remains to find a "rotation" in the three remaining coordinate planes that leaves the interval invariant. Equivalently, to find a way to assign coordinates so that they coincide with the coordinates corresponding to a moving frame.
The general problem is to find a transformation such that
To solve the general problem, one may use the knowledge about invariance of the interval of translations and ordinary rotations to assume, without loss of generality,][ that the frames and are aligned in such a way that their coordinate axes all meet at and that the and axes are permanently aligned and system has speed along the positive . Call this the ''standard configuration''. It reduces the general problem to finding a transformation such that
The standard configuration is used in most examples below. A ''linear'' solution of the simpler problem
solves the more general problem since coordinate ''differences'' then transform the same way. Linearity is often assumed or argued somehow in the literature when this simpler problem is considered. If the solution to the simpler problem is ''not'' linear, then it doesn't solve the original problem because of the cross terms appearing when expanding the squares.
]
The solutions
As mentioned, the general problem is solved by translations in spacetime. These do not appear as a solution to the simpler problem posed, while the boosts do (and sometimes rotations depending on angle of attack). Even more solutions exist if one ''only'' insist on invariance of the interval for lightlike separated events. These are nonlinear conformal ("angle preserving") transformations. One has
Some equations of physics are conformal invariant, e.g. the Maxwell's equations
Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, Electrical network, electr ...
in source-free space, but not all. The relevance of the conformal transformations in spacetime is not known at present, but the conformal group in two dimensions is highly relevant in conformal field theory and statistical mechanics
In physics, statistical mechanics is a mathematical framework that applies statistical methods and probability theory to large assemblies of microscopic entities. Sometimes called statistical physics or statistical thermodynamics, its applicati ...
. It is thus the Poincaré group that is singled out by the postulates of special relativity. It is the presence of Lorentz boosts (for which velocity addition is different from mere vector addition that would allow for speeds greater than the speed of light) as opposed to ordinary boosts that separates it from the Galilean group of Galilean relativity. Spatial rotations, spatial and temporal inversions and translations are present in both groups and have the same consequences in both theories (conservation laws of momentum, energy, and angular momentum). Not all accepted theories respect symmetry under the inversions.
Using the geometry of spacetime
Landau & Lifshitz solution
These three hyperbolic function formulae (H1–H3) are referenced below:
#
#
#
The problem posed in standard configuration for a boost in the , where the primed coordinates refer to the ''moving'' system is solved by finding a ''linear'' solution to the simpler problem
The most general solution is, as can be verified by direct substitution using (H1),
To find the role of in the physical setting, record the progression of the origin of , i.e. . The equations become (using first ),
Now divide:
where was used in the first step, (H2) and (H3) in the second, which, when plugged back in (), gives
or, with the usual abbreviations,
This calculation is repeated with more detail in section hyperbolic rotation.
Hyperbolic rotation
The Lorentz transformations can also be derived by simple application of the special relativity postulates and using hyperbolic identities.
;Relativity postulates
Start from the equations of the spherical wave front of a light pulse, centred at the origin:
which take the same form in both frames because of the special relativity postulates. Next, consider relative motion along the ''x''-axes of each frame, in standard configuration above, so that ''y'' = ''y''′, ''z'' = ''z''′, which simplifies to
;Linearity
Now assume that the transformations take the linear form:
where ''A'', ''B'', ''C'', ''D'' are to be found. If they were non-linear, they would not take the same form for all observers, since fictitious forces (hence accelerations) would occur in one frame even if the velocity was constant in another, which is inconsistent with inertial frame transformations.
Substituting into the previous result:
and comparing coefficients of , , :
;Hyperbolic rotation:
The equations suggest the hyperbolic identity
Introducing the rapidity
In special relativity, the classical concept of velocity is converted to rapidity to accommodate the limit determined by the speed of light. Velocities must be combined by Einstein's velocity-addition formula. For low speeds, rapidity and velo ...
parameter as a hyperbolic angle allows the consistent identifications
where the signs after the square roots are chosen so that and increase if and increase, respectively. The hyperbolic transformations have been solved for:
If the signs were chosen differently the position and time coordinates would need to be replaced by and/or so that and increase not decrease.
To find how relates to the relative velocity, from the standard configuration the origin of the primed frame is measured in the unprimed frame to be (or the equivalent and opposite way round; the origin of the unprimed frame is and in the primed frame it is at ):
and hyperbolic identities leads to the relations between , , and ,
From physical principles
The problem is usually restricted to two dimensions by using a velocity along the ''x'' axis such that the ''y'' and ''z'' coordinates do not intervene, as described in standard configuration above.
Time dilation and length contraction
The transformation equations can be derived from time dilation
Time dilation is the difference in elapsed time as measured by two clocks, either because of a relative velocity between them (special relativity), or a difference in gravitational potential between their locations (general relativity). When unsp ...
and length contraction
Length contraction is the phenomenon that a moving object's length is measured to be shorter than its proper length, which is the length as measured in the object's own rest frame. It is also known as Lorentz contraction or Lorentz–FitzGerald ...
, which in turn can be derived from first principles. With and representing the spatial origins of the frames and , and some event , the relation between the position vectors (which here reduce to oriented segments , and ) in both frames is given by:
Using coordinates in and in for event M, in frame the segments are , and (since is as measured in ):
Likewise, in frame , the segments are (since is ''as measured in'' ), and :
By rearranging the first equation, we get
which is the space part of the Lorentz transformation. The second relation gives
which is the inverse of the space part. Eliminating between the two space part equations gives
that, if , simplifies to:
which is the time part of the transformation, the inverse of which is found by a similar elimination of :
Spherical wavefronts of light
The following is similar to that of Einstein.
As in the Galilean transformation
In physics, a Galilean transformation is used to transform between the coordinates of two reference frames which differ only by constant relative motion within the constructs of Newtonian physics. These transformations together with spatial rotati ...
, the Lorentz transformation is linear since the relative velocity of the reference frames is constant as a vector; otherwise, inertial forces would appear. They are called inertial or Galilean reference frames. According to relativity no Galilean reference frame is privileged. Another condition is that the speed of light must be independent of the reference frame, in practice of the velocity of the light source.
Consider two inertial frames of reference ''O'' and ''O''′, assuming ''O'' to be at rest while ''O''′ is moving with a velocity ''v'' with respect to ''O'' in the positive ''x''-direction. The origins of ''O'' and ''O''′ initially coincide with each other. A light signal is emitted from the common origin and travels as a spherical wave front. Consider a point ''P'' on a spherical wavefront
In physics, the wavefront of a time-varying ''wave field (physics), field'' is the set (locus (mathematics), locus) of all point (geometry), points having the same ''phase (waves), phase''. The term is generally meaningful only for fields that, a ...
at a distance ''r'' and ''r''′ from the origins of ''O'' and ''O''′ respectively. According to the second postulate of the special theory of relativity the speed of light
The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
is the same in both frames, so for the point ''P'':
The equation of a sphere in frame ''O'' is given by
For the spherical wavefront
In physics, the wavefront of a time-varying ''wave field (physics), field'' is the set (locus (mathematics), locus) of all point (geometry), points having the same ''phase (waves), phase''. The term is generally meaningful only for fields that, a ...
that becomes
Similarly, the equation of a sphere in frame ''O''′ is given by
so the spherical wavefront satisfies
The origin ''O''′ is moving along ''x''-axis. Therefore,
must vary linearly with and . Therefore, the transformation has the form
For the origin of ''O''′ and are given by
so, for all ,
and thus
This simplifies the transformation to
where is to be determined. At this point is not necessarily a constant, but is required to reduce to 1 for .
The inverse transformation is the same except that the sign of is reversed:
The above two equations give the relation between and as: